Nuclear physics problems for accreting neutron stars

Details Nuclear physics problems for accreting neutron stars Nuclear physics problems for accreting neutron stars

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aipc..115..319w&link_type=abstract

AIP Conference Proceedings, Volume 115, pp. 319-324 (1984).

Physics

13

Elementary Particle Processes, Neutron Stars, X-Ray Sources, X-Ray Bursts

Scientific paper

The importance of p(e-ν)n and of (p,γ) reactions on 56Ni during
a thermonuclear runaway on a neturon star surface is pointed out. A fast
16-isotope approximate nuclear reaction network is developed that is
suitable for use in hydrodynamic calculations of such events.

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